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The sensitivity of three lines to AR

Published online by Cambridge University Press:  14 March 2005

V. Penza
Affiliation:
INAF - Osservatorio Astronomico di Roma, Via Frascati 33, I-00040, Monte Porzio Catone, Rome, Italy email: penza@mporzio.astro.it
D. Del Moro
Affiliation:
Dip. di Fisica, Universitá “Tor Vergata”, Via della Ricerca Scientifica 1, I-00133, Rome, Italy
B. Caccin
Affiliation:
Dip. di Fisica, Universitá “Tor Vergata”, Via della Ricerca Scientifica 1, I-00133, Rome, Italy
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Abstract

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We study the sensitivity to AR of three photospheric lines, comparing experimental results, from THEMIS observations, with spectral synthesis, demonstrating the inappropriateness of using these lines as indicators of quiet sun modifications, because their variations in the active regions. We try to reconstruct the cyclic lines behavior.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Copyright
© 2004 International Astronomical Union